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Volume 116, Issue 16

22 April 2016
On the Cover

Numerical simulations showing the spatial structure of the dynamo magnetic field generated for a fluid astrophysical object. The colored sphere indicates the amplitude of the radial magnetic field at the surface of the core-mantle boundary. The lines indicate the magnetic field in the insulating mantle and outside of the astrophysical object.

From the article:

Fluctuations of Electrical Conductivity: A New Source for Astrophysical Magnetic Fields
F. Pétrélis, A. Alexakis, and C. Gissinger
Phys. Rev. Lett. 116, 161102 (2016)

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